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蛋白质动力学中的谐性与非谐性:正规模式分析与主成分分析

Harmonicity and anharmonicity in protein dynamics: a normal mode analysis and principal component analysis.

作者信息

Hayward S, Kitao A, Go N

机构信息

Department of Chemistry, Faculty of Science, Kyoto University, Japan.

出版信息

Proteins. 1995 Oct;23(2):177-86. doi: 10.1002/prot.340230207.

Abstract

A comparison of a normal mode analysis and principal component analysis of a 200-ps molecular dynamics trajectory of bovine pancreatic trypsin inhibitor in vacuum has been made in order to further elucidate the harmonic and anharmonic aspects in the dynamics of proteins. An anharmonicity factor is defined which measures the degree of anharmonicity in the modes, be they principal modes or normal modes, and it is shown that the principal mode system naturally divides into anharmonic modes with peak frequencies below 80 cm-1, and harmonic modes with frequencies above this value. In general the larger the mean-square fluctuation of a principal mode, the greater the degree of anharmonicity in its motion. The anharmonic modes represent only 12% of the total number of variables, but account for 98% of the total mean-square fluctuation. The transitional nature of the anharmonic motion is demonstrated. The results strongly suggest that in a large subspace, the free energy surface, as probed by the simulation, is approximated by a multi-dimensional parabola which is just a rescaled version of the parabola corresponding to the harmonic approximation to the conformational energy surface at a single minimum. After 200 ps, the rescaling factor, termed the "normal mode rescaling factor," has apparently converged to a value whereby the mean-square fluctuation within the subspace is about twice that predicted by the normal mode analysis.

摘要

为了进一步阐明蛋白质动力学中的谐波和非谐波方面,对真空条件下牛胰蛋白酶抑制剂200皮秒分子动力学轨迹的正常模式分析和主成分分析进行了比较。定义了一个非谐性因子,用于测量模式(无论是主模式还是正常模式)中的非谐性程度,结果表明主模式系统自然地分为峰值频率低于80厘米-1的非谐模式和频率高于此值的谐波模式。一般来说,主模式的均方涨落越大,其运动中的非谐性程度就越大。非谐模式仅占变量总数的12%,但占总均方涨落的98%。证明了非谐运动的过渡性质。结果强烈表明,在一个大的子空间中,模拟所探测的自由能表面近似于一个多维抛物线,它只是对应于在单个最小值处构象能量表面的谐波近似的抛物线的重新缩放版本。200皮秒后,称为“正常模式重新缩放因子”的重新缩放因子显然已收敛到一个值,由此子空间内的均方涨落约为正常模式分析预测值的两倍。

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